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Perturbation Theory - Advanced Quantum Chemistry and Spectroscopy - Lecture Slides, Slides of Chemistry

Perturbation Theory, the Degenerate Set, General Observations, Solved By Diagonalizing, Static Perturbation, Set Up the Problem, Substitute Expansion, Reasonable Choices, Electronic Transitions Or Vibrational Transitions and few other describes importance of this lecture in Advanced Quantum Chemistry and Spectroscopy course.

Typology: Slides

2011/2012

Uploaded on 11/21/2012

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Download Perturbation Theory - Advanced Quantum Chemistry and Spectroscopy - Lecture Slides and more Slides Chemistry in PDF only on Docsity! โˆ‘ โ‰  โˆ’ >< = qk kq qk q EE H E )0()0( 2)0()1()0( )2( |ห†| ฯ†ฯˆ k is not part of the degenerate set ( ) 2.0 5 1 10 2 10 2 20 10 2 1 2 1 3020 2 1|ห†| 22 )1( 32 )1( 31 2 )0( 2 )0( 1 )1()0( 3 )0( 3 )0( 1 2)1( 31)2( 1 โˆ’=โˆ’=โˆ’= โˆ’ + = โˆ’ + = โˆ’ >+< = โˆ’ =โˆด HH H EE H E ฯˆฯˆฯˆ ( ) 2.0 5 1 10 2 10 2 20 10 2 1 2 1 3020 2 1|ห†| 22 )1( 32 )1( 31 2 )0( 2 )0( 1 )1()0( 3 )0( 3 )0( 2 2)1( 32)2( 2 โˆ’=โˆ’=โˆ’= โˆ’ โˆ’ = โˆ’ โˆ’ = โˆ’ >โˆ’< = โˆ’ =โˆด HH H EE H E ฯˆฯˆฯˆ docsity.com ( ) ( ) 4.0 10 4 10 2 2 10 2 2 10 2 1 2 1 10 2 1 2 1 2030 |ห†| 2 1 2030 |ห†| 2 1 222 )1( 23 )1( 13 2 )1( 23 )1( 13 2 )0( 3 )1()0( 2 )0( 1 2 )0( 3 )1()0( 2 )0( 1 )0( 2 )0( 3 2)1( 23 )0( 1 )0( 3 2)1( 13)2( 3 == โˆ’ += โˆ’ + + = โˆ’ >โˆ’< + โˆ’ >+< = โˆ’ + โˆ’ =โˆด HHHH HH EE H EE H E ฯˆฯˆฯˆฯˆฯˆฯˆ Summary: 4.304.0030 8.182.0120 8.202.0120 )2( 3 )1( 3 )0( 33 )2( 2 )1( 2 )0( 22 )2( 1 )1( 1 )0( 11 =++=++= =โˆ’โˆ’=++= =โˆ’+=++= EEEE EEEE EEEE docsity.com To solve this we substitute expansion into time-dependent Schrodinger Equation and solve for selected initial conditions. Reasonable choices: at t = 0 all molecules are in a particular state j. i.e. ak (o) =ฮดkj ; that is, aj (0) =1; akโ‰ j (0)=0. This makes sense for electronic transitions or vibrational transitions where the Boltzmann Distributions: ( ) kT EE g e ge e N N โˆ’โˆ’ โ‰ˆExcited state population Ground state population ~ 10-16 โ€“ 10-160 ~ 0 Therefore, Ng >> Ne (Note: not necessarily true for rotational energy levels at room temperature). docsity.com c) Exact Solution Preamble: dot convention for time derivatives: .;;; 3 3 2 2 etcf t ff t ff t f โ€ขโ€ขโ€ขโ€ขโ€ขโ€ข = โˆ‚ โˆ‚ = โˆ‚ โˆ‚ = โˆ‚ โˆ‚ Therefore we can write the time dependent Schrodinger wave equation as: ( ) ( ) ( )tr i trtH ,,ห† rhr โ€ข ฮฉโˆ’=ฮฉ ( )( ) ( ) ( ) ( ) ( ) t trta i trtatHH k k k k โˆ‚ โŽฅ โŽฆ โŽค โŽข โŽฃ โŽก โˆ‚ โˆ’=โŽฅ โŽฆ โŽค โŽข โŽฃ โŽก +โ‡’ โˆ‘ โˆ‘ โˆž = โˆž = 1 1 )1()0( , ,ห†ห† r hr ฯ† ฯ† ( ) ( ) ( ) ( ) โˆ‘โˆ‘โˆ‘ โˆž = โˆ’ โˆž = โˆž = โˆ‚ โŽฅ โŽฅ โŽฆ โŽค โŽข โŽข โŽฃ โŽก โˆ‚ โˆ’=+โ‡’ 1 )1( 1 )0( 1 )0( ห†ห† k tiE kk k k kk k k t eta i tHtaHta k h h ฯˆ ฯ†ฯ† Derivation ahead docsity.com
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